Calculations of the Dynamo Coefficients in Galactic Magnetic Fields with Shear

Details Calculations of the Dynamo Coefficients in Galactic Magnetic Fields with Shear Calculations of the Dynamo Coefficients in Galactic Magnetic Fields with Shear

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004assl..315..303o&link_type=abstract

How Does the Galaxy Work? A Galactic Tertulia with Don Cox and Ron Reynolds. Edited by Emilio J. Alfaro, Instituto de Astrofica

Astronomy and Astrophysics

Astrophysics

Scientific paper

We study a three-dimensional (3D) numerical model of the Parker instability in a galactic disk and compute the components of the kinetic and magnetic parts of the dynamo hat α tensor. We find that magnitude of the sum of both parts coincides well with the efficiency of generation of poloidal magnetic field during the growth phase of the Parker instability in differentially rotating disks.

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